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Thursday, May 2, 2019
Wednesday, May 1, 2019
A MORE ACCURATE TWEAK FOR CRISPR.
A Deceptively Simple Tweak to CRISPR Makes It 50 Times More Accurate
CRISPR may be the premiere gene editing progeny poised to upend natural genomes and erase inherited diseases. But since its inception, one thing has always stood in the way: accuracy.
Back in 2017, a contentious report using CRISPR found massive off-target edits in mice, in which the tool went rogue to snip away at innocent genes. Although the study was heatedly refuted and eventually retracted, fears about the powerful tool’s off-target mutations remain. Even CRISPR base-editors, alternate versions that swap one DNA letter with another and are considered relatively accurate, recently came under fire for causing hundreds of unintended mutations in both DNA and RNA.
Without ensuring high levels of accuracy, any proposed CRISPR gene therapy becomes a genetic crapshoot.
Now, a team from Duke University may have found a universal workaround—a trick to fundamentally boost CRISPR’s accuracy in almost all its forms. Published this month in Nature Biotechnology, the team’s study tweaked the design of guide RNAs, the indispensable targeting “blood hound” of the CRISPR duo that hunts down specific DNA sequences before its partner Cas makes the cut.
The upgrade is deceptively simple: tag a “locking” structure to one end of the guide RNA so that only the targeted DNA can unleash the power of the Cas scissors. Yet exactlybecause the tweak is so easy, guide RNA 2.0 can fundamentally tune the accuracy of multiple CRISPR systems—not just those relying on the classic Cas9, but also newer diagnostic systems that deploy Cas12a and other flavors—by as much as 200-fold.
This isn’t another incremental tweak. Rather, the strategy radically differs from previous efforts at boosting CRISPR accuracy, which generally involve fishing for new and better versions of Cas scissors.
“We’re focused on a solution that doesn’t add more parts and is general to any kind of CRISPR system,” said study author Dewran Kocak.
“It’s a nice, elegant solution for getting rid of off-target activity,” added lead author Dr. Charles Gersbach.
Hello, I’m Guide RNA
Why would altering the molecular bloodhound fundamentallyincrease CRISPR accuracy?
There’s historical precedence in the power of RNA structure: the Nobel prize-winning gene silencing technology RNAi, for example, took decades to reveal that minor tweaks to the targeting RNA can greatly reduce immune responses or increase efficiency and accuracy.
These hard-earned lessons from RNAi can inform gene editing. When we describe the CRISPR process, it often goes something like this: the guide RNA—looking like a wriggly worm—contains a letter sequence that matches with the targeted DNA. When the two bind, following a strict marital rule of A to T* and C to G, the guide RNA then drags over Cas scissors and voilà—a nice, clean DNA snip at the intended site. (*More precisely, “T” in DNA and “U” in RNA. Same thing, different names. Thanks history!)
Unfortunately, theory often doesn’t match up with reality in biology. Guide RNA actually looks like multiple clover leaves strung together, packed with bulges—dubbed “stem-loops”—that keep its structure stable and maximize binding efficiency. In all, most guide RNAs only contain 20 or so letters. In a sea of roughly six billion DNA letters in humans, the chance of an unintended partial mismatch is pretty darn high.
This is partly why designing guide RNAs is both a science and an art: unlike Yoda’s famous maxim, “do or do not, there is no try,” scientists often have to repeatedly tinker with their specific guide RNA sequence before it works as intended.
Nevertheless, CRISPR has always had a recipe book for engineering guide RNAs—a general, prototypical design that underlies most CRISPR applications. That’s what the Duke team overhauled.
All About Energy
The team’s inspiration came from cellular energetics.
Like any other biological event, guide RNA binding to DNA and unleashing Cas takes energy. Previous studies found that the more precise the guide RNA-DNA match, the easier it is for the two partners to form a so-called “R loop”: a molecular hybrid that kicks off the whole dicing process.
The team’s brilliant idea is to add an additional clover-like structure to the tail end of the guide RNA. This “hairpin” acts like a physical block in many cases: unless the RNA matches with the targeted DNA, its bulky structure prevents the RNA-DNA pair from forming R-loops. No loops, no cutting, and off-target DNA sequences remain nice and safe.
But if the sequence does match up, the guide RNA, in forming the R-loop with its matching DNA, tears open the hairpin, which in turn spurs Cas scissors into action.
Using computer simulation to guide their designs, the team engineered a whole slew of hairpin guide RNAs, or “hp-sgRNAs” to try out in human cells. When paired with the classic Cas9, the new bloodhounds increased targeting specificity by roughly 50 fold. In one sensitive assay looking at off-target effects throughout the cell’s genome, the team found that compared to classic guide RNAs, their upgraded version eliminated 124 off-target sites and didn’t generate any new ones.
The results were just as impressive with other Cas scissors, many of which only weakly resemble Cas9 in structure and in the way they function. Yet when tag-teamed with the new hairpin guide RNA, Cas12 and its variants were able to cut designated DNA sequences with similar efficiency to when partnering with normal guide RNAs, but with far fewer off-target effects.
What’s more, the team found that they were able to fine-tune the strength of Cas scissors by minutely changing the structure of the hairpin. A “tighter” hairpin made for a stronger lock, which decreased editing efficacy but also dramatically boosted accuracy. A “loser” hairpin helped retain Cas activity, but wasn’t as effective for accuracy.
“By looking at R-loop formation we were able to predict the power of our hairpin guide RNAs,” the authors explained. This predictability is gold—it makes it easier for future scientists to carefully calibrate the strength and accuracy of the hairpin guide RNAs and CRISPR system.
A Changed Recipe
This isn’t the first time scientists have tried boosting CRISPR accuracy.
One previous idea is to make the CRISPR system a ménage à trois: a guide RNA plus two Cas scissors. For DNA cutting to happen, both Cas copies have to bind to the same DNA sequence. Although it’s a clever trick that works, the idea requires scientists to pump more components into the cell, adding further complexity to an already sensitive ecosystem.
Another idea, neutering Cas scissors to make them less likely to jump ship, also had its downfalls. Engineering specific traits into proteins is extremely difficult and time-consuming, and scientists would have to tailor each Cas variant to their needs.
“Doing extensive re-engineering every time we find a new CRISPR protein to make it more accurate is not a straightforward solution,” explained Gersbach.
In contrast, the Duke team’s insight into guide RNAs could radically change the design of CRISPR systems going forward.
“What’s common to all CRISPR systems is the guide RNA, and these short RNAs are much easier to engineer,” said Kocak.
Going forward, the team wants to further confirm that their hairpin guide RNA alternative can work with other Cas scissors already in use. They also want to dig into how the partnership works, and potentially unlock ways to further boost targeting accuracy—not just in free-floating cells, but more importantly, in animal models of genetic diseases.
Image Credit: Meletios Verras / Shutterstock.com
Tuesday, April 23, 2019
A MAGNIFICENT BREAK THROUGH!
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Thursday, April 18, 2019
Helium Hydride found in space.
We Found the Universe’s First Type of Molecule
For decades, astronomers searched the cosmos for what is thought to be the first kind of molecule to have formed after the Big Bang. Now, it has finally been found. The molecule is called helium hydride. It’s made of a combination of hydrogen and helium. Astronomers think the molecule appeared more than 13 billion years ago and was the beginning step in the evolution of the universe. Only a few kinds of atoms existed when the universe was very young. Over time, the universe transformed from a primordial soup of simple molecules to the complex place it is today — filled with a seemingly infinite number of planets, stars and galaxies. Using SOFIA, the world’s largest airborne observatory, scientists observed newly formed helium hydride in a planetary nebula 3,000 light-years away. It was the first ever detection of the molecule in the modern universe. Learn more about the discovery:
Helium hydride is created when hydrogen and helium combine.
Since the 1970s, scientists thought planetary nebula NGC 7027—a giant cloud of gas and dust in the constellation Cygnus—had the right environment for helium hydride to exist.
But space telescopes could not pick out its chemical signal from a medley of molecules.
Enter SOFIA, the world’s largest flying observatory!
By pointing the aircraft’s 106-inch telescope at the planetary nebula and using a tool that works like a radio receiver to tune in to the “frequency” of helium hydride, similar to tuning a radio to a favorite station…
…the molecule’s chemical signal came through loud and clear, bringing a decades-long search to a happy end.
The discovery serves as proof that helium hydride can, in fact, exist in space. This confirms a key part of our basic understanding of the chemistry of the early universe, and how it evolved into today’s complexity. SOFIA is a modified Boeing 747SP aircraft that allows astronomers to study the solar system and beyond in ways that are not possible with ground-based telescopes. Find out more about the mission at www.nasa.gov/SOFIA
Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com
What NASA learned from the twins.
Two are Better Than One: The NASA Twins Study
What exactly happens to the human body during spaceflight? The Twins Study, a 340-day investigation conducted by NASA’s Human Research Program , sought to find answers. Scientists had an opportunity to see how conditions on the International Space Station translated to changes in gene expression by comparing identical twin astronauts: Scott Kelly who spent close to a year in space and Mark Kelly who remained on Earth.
The Process
From high above the skies, for almost a year, astronaut Scott Kelly periodically collected his own blood specimens for researchers on the ground during his One-Year Mission aboard the Space Station. These biological specimens made their way down to Earth onboard two separate SpaceX Dragon vehicles. A little bit of Scott returned to Earth each time and was studied by scientists across the United States.
Totaling 183 samples from Scott and his brother, Mark, these vials helped scientists understand the changes Scott’s body underwent while spending a prolonged stay in low Earth orbit.
The Twins
Because identical twins share the same genetic makeup, they are very similar on a molecular level. Twin studies provide a way for scientists to explore how our health is impacted by the environment around us.
What We Learned: Gene Expression
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